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EUCLIPSE First Period Report

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Compositing methods<br />

- Climatology of Midlatitude Storminess, allowing to composite cloud properties in the<br />

area of influence of midlatitude storms<br />

http://gcss-dime.giss.nasa.gov/mcms/mcms.html<br />

− Tropical El Niño Southern Oscillation Anomaly Database:<br />

http://gcss-dime.giss.nasa.gov/ARRA/arra.html<br />

It must be noted here that the evaluation toolkit will be continuously updated during<br />

the lifetime of the project, as corrections to the existing methods will be applied and<br />

new methods will be created.<br />

WP1.3. Planning, Organization, and Archival of ESM simulations<br />

<strong>EUCLIPSE</strong> ESMs have been performing a hierarchy of experiments, in particular those<br />

proposed by CFMIP-2 as part of the CMIP-5 coordinated experiments. The initial suite<br />

of <strong>EUCLIPSE</strong> climate experiments was performed in the context of WP1. Models are<br />

been run with atmosphere-only configurations and with prescribed Sea Surface<br />

Temperature (SST) patterns. The experiments include: a) Control AMIP simulations<br />

using interannually varying observed SSTs, b) ‘Hansen’ CO2 forcing experiments with<br />

SSTs from the control run and 4xCO2, c) SST perturbation experiments using a<br />

pattern based on a composite of CMIP3 AOGCM CO2 quadrupling experiments, d)<br />

uniform +4K SST perturbations e) Aqua-planet experiments using an idealised zonal<br />

mean climatology for the control, with 4xCO2 and uniform +4K perturbation<br />

experiments. In addition to those runs that are the focus of the CFMIP and <strong>EUCLIPSE</strong><br />

programs, WP1 participants coordinated and monitored the progress of the rest of the<br />

CMIP-5 experiments performed by the participating modelling groups.<br />

Additional diagnostics have been implemented within <strong>EUCLIPSE</strong> ESM model runs. One<br />

primary set of such diagnostics is the output from the COSP simulator. The set of<br />

simulator output variables for short periods (1-3 years) includes a lightweight set of<br />

basic simulator diagnostics, but in addition requires joint height-reflectivity<br />

distribution of CloudSat radar outputs, joint height-lidar scattering ratio distribution of<br />

lidar outputs, as well as cloud frequency of occurrence as seen by CALIPSO but not<br />

CloudSat, required for studies making combined use of CloudSat/CALIPSO simulator<br />

output.<br />

For a 1-year period of the AMIP control experiment, 3-hourly global instantaneous<br />

outputs are produced. These experiments will allow the process modelling groups in<br />

WP3 to examine the representation of cloud processes by GCMs in the current climate<br />

in any climate regime or meteorological situations without imposing a priori<br />

geographical constraints. In addition, for several years of the AMIP control run, 3hourly<br />

outputs are produced along a few transects (e.g. GCSS/WGNE-Pacific Crosssection<br />

Intercomparison - GPCI, VOCALS) or locations for which a large number of<br />

observations will be available (satellite data for GPCI, field campaign for VOCALS,<br />

long-time series of ground-based observations for ARM or CloudNet instrumented<br />

sites).<br />

WP1 has been closely monitoring the progress of both CFMIP-specific and CMIP-5 runs<br />

through regular submissions of progress reports by the different partners. As a result,<br />

13

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